69-92 hoofdstuk 4 - COnnecting REpositoriesCH 4 emission at the site over 2005 and 2006 was...
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An eddy covariance set-up for methane measurements
69
4444
A compact and stable eddy covariance set-up
for methane measurements
using off-axis integrated cavity output spectroscopy
This chapter was published as Hendriks, D.M.D., Dolman, A.J., Van der Molen, M.K.,
Van Huissteden, J., 2008. A compact and stable eddy covariance set-up for methane
measurements using off-axis integrated cavity output spectroscopy. Atmos. Chem. Phys.
8, 431-443.
Abstract
A Fast Methane Analyzer (FMA) is assessed for its applicability in a closed path eddy
covariance field set-up in a peat meadow. The FMA uses off-axis integrated cavity output
spectroscopy combined with a highly specific narrow band laser for the detection of CH4
and strongly reflective mirrors to obtain a laser path length of 2-20×103 m. Statistical
testing and a calibration experiment showed high precision (7.8×10-3
ppb) and accuracy (<
0.30%) of the instrument, while no drift was observed. The instrument response time was
determined to be 0.10 s. In the field set-up, the FMA is attached to a scroll pump and
combined with a 3-axis ultrasonic anemometer and an open path infrared gas analyzer for
measurements of carbon dioxide and water vapour. The power-spectra and co-spectra of
the instruments were satisfactory for 10Hz sampling rates.
Due to erroneous measurements, spikes and periods of low turbulence the data series
consisted for 26% of gaps. Observed CH4 fluxes consisted mainly of emission, showed a
diurnal cycle, but were rather variable over time. The average CH4 emission was 29.7
nmol m-2
s-1
, while the typical maximum CH4 emission was approximately 80.0 nmol m-2
s-1
and the typical minimum flux was approximately 0.0 nmol m-2
s-1
. The correspondence
of the measurements with flux chamber measurements in the footprint was good and the
observed CH4 emission rates were comparable with eddy covariance CH4 measurements
in other peat areas.
Additionally, three measurement techniques with lower sampling frequencies were
simulated, which might give the possibility to measure CH4 fluxes without an external
pump and save energy. Disjunct eddy covariance appeared to be the most reliable
substitute for 10Hz eddy covariance, while relaxed eddy accumulation gave reliable
estimates of the fluxes over periods in the order of days or weeks.
Chapter 4
70
4.1 Introduction
Methane is the third most important greenhouse gas globally, after water vapour and
carbon dioxide. Its concentration has risen by 150% since the pre-industrial era (Foster et
al., 2007) and currently 20% of the enhanced greenhouse effect is considered to be due to
methane (Foster et al., 2007). Although methane is less abundant in the atmosphere
compared to carbon dioxide, it is a relatively strong greenhouse gas: the Global Warming
Potential of methane expressed as CO2-equivalents is approximately 25 (over 100 years)
while that of carbon dioxide is by definition 1 (Foster et al., 2007). For water vapour and
carbon dioxide, the eddy covariance technique has been used for several decennia
(Aubinet et al., 2000) to measure the exchange of these gases with the earth surface. In
eddy covariance, the vertical flux (Fs) of an atmospheric property (s) is directly
determined by the covariance of that property and the vertical velocity, as shown in Eq.
(4.1). This can be obtained by calculating the time averaged product (over the period t1 to
t2) of the deviation (s’) of the atmospheric property (s), from 'sss += , and the deviation
(w’) of the vertical wind velocity (w) from 'www += :
∫−
==
2
112
)(')('1
''
t
t
s dttstwtt
swF (4.1)
(Aubinet et al., 2000). The eddy covariance technique requires an instrument with high
precision, accuracy and system stability as well as high sampling rates and short
instrument response time (τ). Unfortunately, the low abundance of methane in the
atmosphere hampers adequate concentration measurements of this gas and the eddy
covariance technique has therefore been rarely applied for the assessment of methane
emissions (Kroon et al., 2007; Hargreaves et al., 2001; Kormann et al., 2001). The
advantages of the eddy covariance technique compared to other techniques for measuring
trace gases are nonetheless obvious: integrated continuous measurements over a large
footprint area (102 to 10
4 m
2) and longer periods without disturbance from small scale
surface features. These properties enable assessments of spatial and temporal variability at
the landscape scale.
Since the 1980s, infrared absorption spectrometry using tunable diode lasers (TDLs) has
been widely used for measurements of trace gases in the lab. A field technique for eddy
covariance using a multipass absorption cell was introduced in 1995 (Zahniser et al.
1995). Unfortunately, serious problems of drift and low sensitivity effects occurred.
Additionally, the method had more practical drawbacks: the large nitrogen Dewar for
temperature control that needs refill weekly, an extensive and sensitive optical module,
and frequent calibration. Improvements were made with the Quantum Cascade Laser
(QCL) spectrometer which was first introduced in 1994 (Faist et al., 1994). The method
was more stable and accurate in eddy covariance set-up than the TDL spectrometry
(Nelson et al., 2004; Kroon et al., 2007), but the practical drawbacks of the methane
instruments (large nitrogen Dewar, optical module, and frequent calibration) were still
present in the QCL spectrometer technique. Hitherto, the micrometeorological
An eddy covariance set-up for methane measurements
71
measurement techniques for methane have thus implied very expensive, large and labour
intensive field set-ups with logistic limitations to unattended field deployment.
The objective of this study was to investigate the applicability and quality of the FMA, a
new off-axis integrated cavity output spectroscopy (ICOS) technique using a highly
specific narrowband laser, for its applicability for eddy covariance field measurements of
methane. The relatively user-friendly and low cost set-up is tested for precision, accuracy
and system stability as well as its’ performance in eddy covariance field set-up. The first
data series are analysed and compared with data obtained by existing measurement
techniques. To asses the applicability of the instrument at locations that lack external
power supply, alternative measurements techniques of the set-up are simulated which
could reduce the power requirements.
4.2 Methods and materials
4.2.1 Instrument design
A measurement cell with highly reflective mirrors was combined with a highly specific
narrowband laser system by O’Keefe et al. (1998), creating a path length of at least two
km in the measurement cell. In this manner, small absorption rates cause much larger
reduction of the total transmitted laser intensity. The ICOS technique could therefore be
used for the detection of gases with ultra weak absorption, while making the extensive
optical module and the nitrogen Dewar superfluous. The operation of the DLT-100 Fast
Methane Analyzer (FMA) from Los Gatos Research Ltd. is based on this improved ICOS
technique and uses a distributed feedback (DFB) diode laser with a wavelength of nearly
1.65 µm. The DFB diode laser offers tunability, narrow line width and high output power
in a compact and very rugged setup. It features a grating structure within the semi-
conductor, which narrows the wavelength spectrum and guarantees single-frequency
emission. Off-axis ICOS implies that a laser beam directed into the measurement cell at a
slight angle, after which it is reflected in the cell numerous times by highly reflective
mirrors (reflectivity ~ 0.9999), thus creating a path length of 2-20×103 m by making 1-
10×104 passes in the cell (Bear et al., 2002; Fig. 4.1). The detector measures fractional
absorption of light at the methane resonant wavelength, which is an absolute measurement
of the methane concentration in the cell.
The path length of the laser, and therefore the time period during which the laser is being
reflected in the cell for each measurement, is dependent on the reflectivity of the mirrors
in the measurement cell. This period over which the laser is being reflected in the
measurement cell is called the mirror ringdown time (MRT) and is continuously
monitored by the FMA. The MRT cannot be allowed to drop below 3.0 to 3.5 µs, since the
laser path length then becomes too short to detect the changes in laser intensity properly.
The mirrors in the measurement cell are sensitive to dirt accumulating in the measurement
cell; a small contamination of the measurement cell causes rapid decrease of the MRT.
Cleaning the mirrors is a relatively simple procedure that can be done in a dust-free
environment.
Chapter 4
72
The FMA measures in the concentration range from 10 to 25×103 ppb and operates
autonomously. Technically, measurements can be made at rates up to 20Hz and at ambient
temperatures of 5 oC to 45
oC, while humidity should be below 95% to avoid
condensation. The pressure in the measurement cell (Pcell), which can be adjusted by a
valve switch on the instrument, should be kept near 210 hPa. To obtain sampling rates
higher then 1Hz, an external pump is needed to maintain the required Pcell and τ.
The measurement cell has a volume of 0.55×10-3
m3 and a length of 0.20 m (Fig. 4.1).
Data output is provided in analogue as well as digital format (RS232&TCP/IP) and the
device can store data up to 10 gigabytes. Warm-up time is approximately one minute and
measurements as well as performance can be observed on a colour TFT LCD flat panel
display. The dimensions of the FMA are 0.25 m height, 0.97 m width and 0.36 m depth
and it has a weight of 22 kg. Power requirements are 115/230 VAC, 50/60Hz and 180W
and inlet/outlet fittings are of the Swagelok type (3/8”,
1/4”).
4.2.2 Site description
Besides testing in the laboratory, the FMA was tested in an eddy covariance set-up at the
Horstermeer measurement site. This site is located in a eutrophic peat meadow area in the
central part of the Netherlands and was described extensively by Hendriks et al. (2007).
The area has a flat topography and vegetation consists of grasses, small shrubs and reeds.
Before, CH4 fluxes in the area were measured with the flux chamber technique and
variation between three land elements was observed: emissions from the saturated land
0.21 m
0.06 m
~0.50 m
0.20 m
Figure 4.1: Schematic overview of the integrated cavity output analysis (ICOS)
technique used in the FMA. (Source: Los Gatos Research Ltd.) “R” is the reflectivity
of the mirrors and “T” and “P” are the sensors of Tcell and Pcell.
An eddy covariance set-up for methane measurements
73
and water surfaces were high compared to the relatively dry land. The annual weighted
CH4 emission at the site over 2005 and 2006 was estimated at 83.95 ± 54.81 nmol m-2
s-1
(Hendriks at al., 2007).
4.2.3 Assessment of instrument stability, precision and accuracy
System stability is a major factor influencing high-sensitivity measurements.
Theoretically, the signal from a perfectly stable system could be averaged infinitely.
However, real systems are stable only for a limited time period. The length of time over
which a laser signal can be averaged to achieve optimum sensitivity, and thus high
precision, largely determines the quality of the spectrometer. The precision of
concentration measurements should be at least a few parts per thousand of the ambient
mixing ratio., which is approximately 4 ppb for a mixing ratio of approximately 1800 ppb
(outside air) in the case of CH4 (Kroon et al., 2007). Both maximum system stability and
precision can be determined using the Allan variance (Allan, 1966; Werle et al., 1993;
Nelson et al., 2004; Kroon et al., 2007). The Allan variance (2
Aσ ), as a function of
integration time Τ, is the average of the sample variance of two adjacent averages of time
series of data and is described by Eq. (4.2):
2
11
2)]()([
2
1)( kAkA
mk s
m
ss
tA −= ∑
=
+σ (4.2)
with: ∑=
++=
k
llkss x
kkA
1)1(
1)( , with: s = 1,…..,m and m = m’ – 1
I
n this equation A is an average of the CH4 concentration, k is the number of elements in
subgroup x, s is the subgroup number, l is the sample-number in the subgroup, and m’ the
number of independent measurements. It is assumed that data are collected over a constant
data interval ∆t, therefore the integration time Τ = k∆t (Allan, 1966; Werle et al., 1993;
Nelson et al., 2004). The Allan variance decreases when random noise dominates over
drift effects. However, when noise caused by instrumental drift of the system starts to
dominate, the Allan variance starts to increase, indicating a decrease of system stability
and hence precision. CH4 concentration measurements over a ten minute period of relative
constant CH4 concentrations with a mean value of 1905 ppb and a standard deviation of
4.74 ppb with 10Hz sampling rate were used to determine the Allan variance.
Subsequently, the Allan variance of this period was plotted over the integration time Τ
(Fig. 4.2), showing a decreasing Allan variance over integration times larger than 2.4 s.
No increase of the Allan variance was observed at larger integration times, indicating an
absence of instrumental drift, and thus high system stability and precision, for integration
times of a few seconds up to ten minutes. Additionally, an indication for the short term
precision (σ) was obtained by the y-axis intercept at the minimum Allan variance (2
Asσ =
6.1×10-3
ppb2). Using Eq. (4.3):
Chapter 4
74
2/1−×= sAs fσσ (4.3)
in which Asσ is the square root of the minimum Allan variance and fs is the sampling
frequency of the system (10Hz), σ was determined as 7.8×10-3
ppb Hz-1/2
. Precisions of
0.3 ppb Hz-1/2
(Nelson et al., 2004) and 2.9 ppb Hz-1/2
(Kroon et al., 2007) were found in
previous studies of QCL instruments.
Next, a calibration experiment was carried out by administering standard gas mixtures
with concentrations of 125 ppb and 2002 ppb CH4, both with an accuracy of 0.2 ppb, to
the FMA at ten instances within a 10-day period. During the whole experiment the FMA
was never turned off in order to imitate longer measurement periods as will be the case in
the field set-up. The deviation from the standard gas values of CH4 (MD) was calculated
for each measurement by Eq. (4.4):
1.82
1.86
1.90
1.94
1.98
0 100 200 300 400 500 600
time (sec)
CH
4 c
oncentr
ation (
ppm
)
1.0E-08
1.0E-07
1.0E-06
1.0E-05
1 10 100 1000integration time (s)
Alla
n V
ariance б
A2 (ppm
2)
a.
b.
Figure 4.2: Time series of CH4 concentration measurements with 10Hz sampling rate with a
mean of 1905 ppb and a standard deviation of 4.74 ppb (a.) and the Allan variance plot for
these data (b.).
An eddy covariance set-up for methane measurements
75
MD = S
SM − (4.4)
where M is the measured CH4 concentration in ppb and S is the CH4 concentration of the
standard gas in ppb. A two-point calibration factor (Fcal) was calculated for each set of
measurements by Eq. (4.5):
Fcal =
LH
LH
MM
SS
−
− (4.5)
where SH and SL are the high and low standard values of CH4 in ppb and MH and ML are
the high and low measured values of CH4 in ppb. Although the measured concentration
sometimes varied one or two ppb from the standard values over the experimental period
for both gases, no actual drift was observed in the instrument (Table 4.1). Fcal was 1.000
on average with fluctuations < 0.30%, indicating high accuracy of the FMA.
Additionally, over a period of a week, CH4 concentration measurements at the
Horstermeer site were compared with CH4 concentrations measured at 20 and 60 m height
at a measurement site in Cabauw (51o58’N and 4
o 55’E)
1, approximately 30 km from the
Horstermeer site. The CH4 concentrations at Cabauw were measured with a Carlo Erba
1 The CH4 concentration measurements in Cabauw are measured with a gas chromatograph by the Energy
Centre of the Netherlands (ECN).
time
date time elapsed M L M H
(days) (ppb) (ppb)
02/04/2007 11:50:00 0.000 125 -0.10% 2005 0.20% 0.998
03/04/2007 09:00:00 0.882 127 1.50% 1999 -0.10% 1.003
03/04/2007 15:30:00 1.153 125 -0.10% 1999 -0.10% 1.002
04/04/2007 09:20:00 2.896 125 -0.10% 2000 -0.10% 1.001
04/04/2007 16:45:00 2.205 125 -0.10% 1999 -0.10% 1.002
05/04/2007 09:30:00 2.903 125 -0.10% 1999 -0.10% 1.002
05/04/2007 17:30:00 3.236 124 -0.90% 2001 0.00% 1.000
10/04/2007 09:45:00 7.913 125 -0.10% 2004 0.10% 0.999
11/04/2007 09:40:00 8.910 125 -0.10% 2002 0.00% 1.000
11/04/2007 16:30:00 9.194 125 -0.10% 2002 0.00% 1.000
12/04/2007 09:15:00 9.892 125 -0.10% 2004 0.10% 0.999
measurement
MD L MD H
Calibration experiment FMA
low CH4 gas (125 ppb) high CH4 gas (2002 ppb)F cal
Table 4.1: Results of the 10-day calibration experiment with two standard gases of 125 and
2002 ppb respectively. Time elapsed since start of experiment, CH4 concentrations measured
by FMA (ML and MH), MD values and Fcal values are shown.
Chapter 4
76
gas chromatograph system and have a precision of 2 ppb. The CH4 concentration at the
Horstermeer site was 15 ppb higher on average, which might be the result of the relatively
high CH4 emissions from the peat meadow area in which the measurements were taken.
Nonetheless, the increasing trend of CH4 concentration at the Horstermeer site was similar
to the trend at the Cabauw site. Generally, slow variation in concentrations is caused by
the difference between continental and marine background concentration, the continental
concentration being approximately 50 ppb higher (Eisma et al., 1994). During the
measurement period, prevailing winds were from the east (continental). This accounted for
the slow rise in CH4 concentrations at both measurement locations.
The influence of changing temperature and pressure conditions in the measurement cell on
CH4 concentration measurements was assessed in the laboratory. During a time series of
continuous measurements, a step change in Pcell was induced, while the temperature in the
measurement cell (Tcell) increased steadily. An effect of the increase of Tcell on CH4
concentration was observed neither from the time series, nor from the correlation plots
(Fig. 4.3). A decrease in the CH4 concentration data was observed 990 sec after the sharp
decrease in Pcel. However, this feature did not result in a clear correlation between CH4
1895
1900
1905
1910
1915
1920
1925
1930
0 0.5 1 1.5 2 2.5time (hours)
CH
4 c
on
c.
(pp
b)
31.2
31.6
32.0
32.4
32.8
0 0.5 1 1.5 2 2.5time (hours)
tem
pe
ratu
re (
oC
)
197
198
199
200
0 0.5 1 1.5 2 2.5
time (hours)
pre
ssu
re (
hP
a)
1895
1900
1905
1910
1915
1920
1925
197.0 197.5 198.0 198.5 199.0 199.5 200.0pressure (hPa)
CH
4 c
on
ce
ntr
atio
n (
pp
b)
1895
1900
1905
1910
1915
1920
1925
31 31.5 32 32.5 33
temperature (oC)
CH
4 c
on
ce
ntr
atio
n (
pp
b)
R2 = 0.00002
R2 = 0.0853
Figure 4.3: Results of the laboratory experiment on the effect of Tcell and Pcell on CH4 concentration
measurements. a.: time series of CH4 concentration measurements; b.: time series of Tcell
measurements; c.: time series of Pcell measurements; d.: scatter plot of CH4 concentration against Tcell
with correlation coefficient (R2); e.: scatter plot of CH4 concentration against Pcell with R
2.
An eddy covariance set-up for methane measurements
77
concentration and Pcell. Also, this type of Pcell changes did not occur under normal
circumstances when Pcell had a stable value near 210 hPa.
4.2.4 Incorporation of FMA in eddy covariance system
After testing in the laboratory, the FMA was installed in a closed-path eddy covariance
field set-up (Fig. 4.4). In order to obtain 10Hz measurements, a dry vacuum scroll pump
(XDS35i, BOC Edwards, Crawly, UK) was used with a maximum pumping speed of
9.72×10-3
m3 s
-1. However, at the required pressure of 210 hPa the actual pumping speed
was 5.50×10-3
m3 s
-1. The scroll pump has relatively high power requirements: 100/200V
to 120/230V, 50/60Hz and 600W. It was placed at the end of the set-up, connected to the
FMA by a wire-reinforced tube with an internal diameter of 1.9×10-3
m, sucking air
through the system. The FMA was placed in a heated, water resistant box, while the scroll
pump was placed in an aerated box that prevented it from getting wet and from
overheating. In addition to the internal filter with a pore size of 2 µm (Swagelok part no.
SS-4FW4-2), a filter with a pore size of 60 µm was placed at the inlet in order to prevent
dust, aerosols, insects and droplets from entering the tubing. The inlet was shielded from
the rain by a stainless steel cap. To prevent any water that accidentally passed the first
filter from moving down toward the analyzer the air was first led up through a stainless
steel tube (diameter of 6.4×10-3
m) that bends sharply at 0.5 m after which the air moves
data from
sonic
anemometer
to handheld
system
data from sonic to
handheld system
1+2
3
4
7
5
8 81011
12
15
direction data
direction air flow
3x25A;
17
14
6
9 16
13
1 rain cap (sharpened at the edges)
2 filter (60 µm)
3 bended tubing of stainless free steel
4 teflon tubing (diameter=64 mm)
5 water locked case
6 tube with warming strip
7 Fast Methane Analyser
8 heating elements
9 sturdy pipe to pump
10 semi closed case
11 scroll pomp
12 air exhaust with silencer
13 3-axis utra sonic anemometer
14 Licor7500 (CO2 and H2O analyser)
15 data collection in Gill software
16 handheld computer
17 power supply (regional electricity network)
swagelok screws are used for all connections
1.20 m
1.00 m 0.70
4.30
1 rain cap (sharpened at the edges)
2 filter (60 µm)
3 bended tubing of stainless steel
4 teflon tubing (diameter=64 mm)
5 water locked case
6 tube with warming strip
7 Fast Methane Analyser
8 heating elements
9 sturdy pipe to pump
10 semi closed case
11 scroll pomp
12 air exhaust with silencer
13 3-axis ultra sonic anemometer
14 Licor7500 (CO2 and H2O analyser)
15 data collection in Gill software
16 handheld computer
17 power supply (regional electricity network)
swagelok screws are used for all connections
Figure 4.4: Schematic overview of the combined field set-up of the closed path eddy
covariance system for CH4 using the FMA and the open path eddy covariance system
for CO2 and water vapour.
Chapter 4
78
down toward the analyzer through a Teflon tube (diameter of 6.4×10-3
m). After the air
has passed through the FMA measurement cell it flows through the scroll pump and was
exhausted through a silencer. The gas-inlet filter was positioned 0.2 m away from the LI-
7500 open path infrared gas analyzer (LI-COR Lincoln, NE, USA) and a Windmaster Pro
3-axis ultrasonic anemometer (GILL Instruments Limited, Hampshire, UK) directed into
the prevailing wind. Both instruments were installed at 4.3 m above the surface at the
Horstermeer measurement site (Hendriks et al., 2007). Data were logged digitally on a
handheld computer at a rate of 10 Hz (Van der Molen et al., 2006).
4.2.5 Assessment of FMA in measuring CH4 fluxes
In general a sampling rate of 10Hz, with a Nyquist frequency of 5Hz, is used for eddy
covariance techniques (Aubinet et al., 2000; Kroon et al. 2007). Therefore an instrumental
time response of 10Hz or greater is required in order to correlate with the wind
measurements made with the 3-axis ultrasonic anemometer. The measurement rate of an
instrument is determined by both electronic signal processing and by the τ of the
measurement cell (Nelson et al., 2004). Electronic signal processing is dependent on the
spectral complexity of the measurement technique as well as the technical design of the
ICOS technique. In the case of the FMA, this was defined by the designers (Los Gatos
Research Ltd.) as 20Hz. The limiting factor of the maximum sampling rate is often τ,
which could be determined by the volume of the measurement cell (0.55×10-3
m3) divided
by the actual pumping speed (5.50×10-3
m3 s
-1) giving a flow response of 0.10 s.
Additionally, τ was determined by applying a step change in concentrations at 20Hz
sampling rate (Fig. 4.5) (Moore, 1986; Zahniser et al., 1995; Nelson et al., 2004). Each
data point was the average mixing ratio of multiple step change events at a certain t (time
elapsed since step change in concentration). The τ was defined by the exponential fit to the
decay of the CH4 mixing ratio and was calculated τ = 0.11 s by Eq. (4.6):
[CH4]t = [CH4]t=0 e (-t/ τ)
(4.6)
0
0.2
0.4
0.6
0.8
1
-0.5 0.0 0.5 1.0 1.5 2.0
time (s)
dC
ob
s/d
Cin
cr
tube length = 0.25m
tube length = 1.00m
Figure 4.5: Averaged and
normalised time series of CH4
concentration data showing
the instrument response with
20Hz sampling rate changing
from ambient air to a gas
sample with a high CH4
concentration for tube lengths
of 0.25 m and 1.0 m.
An eddy covariance set-up for methane measurements
79
10-3
10-2
10-1
100
101
10-3
10-2
10-1
100
n [Hz]
n S
wC
H4
(n)
Observed wCH4
Theoretical w-scalar
10-3
10-2
10-1
100
101
10-3
10-2
10-1
100
n [Hz]
n S
w(n
)
Observed w
Theoretical w
10-3
10-2
10-1
100
10-3
10-2
10-1
n [Hz]
f S
w(n
)
Observed CH4
Theoretical scalar
a.
b.
c.
Figure 4.6: Averaged and binned
results of the spectral analyses of the
FMA eddy covariance set-up for two
moderately turbulent days (six half
hour periods per day). a.: Observed
and theoretical power-spectrum w;
b.: Observed and theoretical power-
spectrum of [CH4]; c.: Observed and
theoretical co-spectrum of w’[CH4]’.
Chapter 4
80
where [CH4]t is the CH4 concentration at instance t. In this, sensitivity to tube length could
be observed (Fig. 4.5). The data in the graph are normalized by the transformation
dCobs/dCincr, where dCobs is the increase of [CH4] between the starting time and time t and
dCincr is difference between the final [CH4] and [CH4] at the starting time. Since the effect
of tube damping was corrected separately, and τ only refers to the response of the
instrument itself, the actual τ was determined as 0.10 s.
The suitability of the FMA eddy covariance set-up was further evaluated by examining the
power spectra of w and [CH4] and co-spectrum of the covariance w’[CH4]’ (Stull et al.,
1988; Kaimal and Finnigan, 1994). For this purpose twelve half hours of data from two
days with moderately unstable conditions were analysed. The results of the spectral
analysis were averaged and binned and the logarithmic spectral and co-spectral densities
were plotted against frequency (Fig. 4.6). Additionally, the theoretical spectra defined by
Kaimal et al. (1972) and Højstrup (1981) were plotted in the graphs (Smeets et al., 1998).
The power spectrum of w very closely followed the whole theoretical spectrum, while
both the [CH4] power spectrum and the w’[CH4]’ co-spectrum showed slight deviations
from the theoretical spectrum. Most important is that the inertial subranges of both the
power spectra and the co-spectrum were in general agreement with the theoretical curve.
The [CH4] power spectrum showed a slight tendency to extend upward in the low
frequency range. This was also observed in the [CO2] power spectrum from the LI-7500
analyzer at the site (Hendriks et al., 2007), indicating that the upward tendency in the low
range was not instrument related, but was rather an effect of environmental factors.
Kaimal et al. (1976) found high densities of low frequencies in the temperature power
spectrum in response to a diurnal cycle. Since a diurnal cycle was observed for both [CO2]
and [CH4] at the Horstermeer site, this might have been the cause of the upward tendency
observed in the power spectra. However, the overestimation of low frequencies will
automatically cause an underestimation of the high frequencies, since the total area under
the power spectrum is a fixed surface (Kaimal et al., 1972; Højstrup, 1981). Considering
the w’[CH4]’ co-spectrum, the observed peak near n=10-1
Hz generally matched the peak
of the theoretical spectrum and was in agreement with spectral analysis of CH4 flux
measurements by Verma et al. (1992), Kormann et al. (2001) and Werle and Kormann
(2001). The spectral performance of the eddy covariance set-up for temperature and CO2
fluxes were discussed previously in a paper by Hendriks et al. (2007) and were in
agreement with the spectral analyses of the CH4 flux measurements.
Additionally, in previous research by Hendriks et al. (2007) the energy balance consisting
of the eddy covariance measurements of latent heat and sensible heat, the micro-
meteorological measurements of incoming and reflected radiation components and the
ground heat flux showed a closure of 82%. This indicated that the data from the eddy
covariance set-up were acceptable (Lloyd et al., 1997).
The travel time of the air in the closed path set-up from the inlet filter to the FMA, caused
a time lag with respect to the in situ measured wind data. For 20 half hour periods, the
covariance w’[CH4]’ of w’ at instance t = 0.0 s and [CH4]’ at t = 0.0 s was determined, as
well as the covariance of w’ at t = 0.0 s and [CH4]’ at the t = 0.1 s, t = 0.2 s, t = 0.3 s, …, t
= 2.0 s. For all half hour periods the highest value of w’[CH4]’ occurred with [CH4]’ at t =
An eddy covariance set-up for methane measurements
81
0.6 s. For the calculation of the actual covariance the time lag of the CH4 measurements
compared to the wind measurements was therefore taken as 0.6 s.
4.2.6 Data processing
The EUROFLUX methodology (Aubinet et al., 2000) was applied to the eddy covariance
data to calculate the CH4 fluxes from the closed path system and the CO2 fluxes from the
open path system (Hendriks et al., 2007) on a thirty minute basis. Since system
instrumental drift was not observed, an overestimation of the fluxes as a result of this
averaging period was not expected. The damping effect of the τ on the CH4 signal was
corrected for in the flux calculation procedure as well as for the time lag of 0.6 s between
closed path CH4 and open path wind, temperature and CO2 measurements (Moore et al.,
1986). The tube length of the set-up was over 1000 times the inner diameter of the tube
and therefore the air temperature in the measurement cell could be considered stable. As a
result, the Webb correction for density fluctuations arising from variations in temperature
that was applied to the open path CO2 measurements, was not required for the closed path
measurements of CH4 (Leuning and Moncrieff, 1990). The Webb correction for density
fluctuations arising from variations in water vapour (measured with the LI-7500) was
applied according to Leuning and Moncrieff (1990). Frequency loss corrections for
closed-path systems were applied according to the theory of Leuning and King (1992).
Since 3-axis ultrasonic anemometers were found to under measure wind speed at large
angles, the method of Nakai et al. (2006) was used to apply the angle of attack dependent
calibration (Gash and Dolman, 2003, Van der Molen et al., 2004).
4.2.7 Simulation of alternative flux measurement approaches
In eddy covariance, the sampling rate determines the number of samples that are taken out
of an infinitely large number of samples. The higher the sampling rate, the higher the
statistical reliability, which results in higher accuracy of the observed means and
covariances (Van der Molen, 2002). In order to obtain reliable estimates of fluxes, a
sampling rate of at least 10Hz is generally used for eddy covariance techniques. However,
measurements performed at lower rates than 10Hz can generate reliable results too (Rinne
et al., 2000 and 2001; Graus et al., 2006; Businger and Oncley, 1990). 1Hz eddy
covariance, disjunct eddy covariance, 1Hz eddy covariance and relaxed eddy
accumulation (REA) are possible alternatives for the preferred 10Hz eddy covariance.
These measurement techniques could make the external pump of the FMA eddy
covariance set-up superfluous and thus save over half of the energy required for the eddy
covariance set-up. This might be necessary for operation in remote places where an
external power source is not available. Here, the raw CH4, CO2 and water vapour 10Hz
field data were manipulated to simulate 1Hz eddy covariance, disjunct eddy covariance
and REA.
With 1Hz eddy covariance, Fs is determined in the same manner as 10Hz eddy covariance
(Eq. (4.2)), but at a lower frequency. The method was tested by averaging each 10
consecutive data points of CH4 concentration as well as wind velocity for the 10Hz data
set, thereby simulating a slower sampling rate (1Hz) with a longer τ (1.0 s instead of 0.10
s).
Chapter 4
82
Disjunct eddy covariance uses a subset of the whole 10 Hz time series to determine the
flux of an atmospheric property Fs according to Eq. (4.7):
∑=
×>==<
N
iiis sw
NswF
1
''1
'' (4.7)
where N is the subset of the data (Rinne et al., 2000 and 2001). Here, the disjunct eddy
covariance method was tested by sampling the first data point of every 10 data points from
the 10Hz data set, thereby creating a time interval of 0.9 s between the sampling moments,
while the τ remained 0.10 s. To build a field set-up for disjunct 1Hz eddy covariance a
‘snap sampling’ instrument would have to be mounted in front of the inlet of the system to
obtain samples that are sampled with a frequency of 1Hz, while maintaining the sampling
duration as short as possible (‘snap’). This method would give the FMA an analysis time
of 1.0 s instead of 0.10 s.
REA is a conditional sampling method in which air samples are drawn into two separate
reservoirs depending on the direction of w. The criterion of valve switching is based on
values of the standard deviation of w ( wσ ), which is measured by the 3-axis ultrasonic
anemometer at 10Hz. The valve is activated according to the threshold
condition ww σ6.00 = . In the case of 00 www ≤≤− (deadband values), neither “up”
nor “down” samples are taken, but samples are discarded from the sampling system
(Graus et al., 2006). Here, we simulated REA by dividing all eddy covariance data points
of one half hour measurement period into three data matrices based on the direction of the
w (upward, downward and deadband values). Next, the measured concentrations are
summed and the turbulent flux of the scalar s (Fs) was determined according to Eq. (4.8):
sbF ws ∆××≈ σ (4.8)
(Businger and Oncley, 1990). The b-value is the correction for the deadband and s∆ the
difference between the concentrations in the accumulation reservoirs (Bowling et al.,
1999).
4.3 Results
4.3.1 First data series
From the eddy covariance data series 11% consisted of gaps due to failure of the eddy
covariance set-up caused by rain events and instrumental errors. Additionally, 3% of the
data series consisted of spikes (CH4 flux > 100.0 nmol m-2
s-1
and CH4 flux < -10.0 nmol
m-2
s-1
) and were removed from the data set. During nighttime periods with low friction
velocity (u*) the turbulence of the atmosphere can become too low for the performance of
eddy covariance measurements (Wohlfahrt et al., 2005; Dolman et al., 2004). In order to
determine the critical u* value for CH4 eddy covariance measurements at this specific site,
the CH4 flux data and u* data from periods with incoming shortwave radiation (SWin) <
An eddy covariance set-up for methane measurements
83
20W m-2
were selected (Dolman et al., 2004). The nightly CH4 fluxes showed a
significant decrease for periods with u* < 0.09 m s-1
(Fig. 4.7). This result is similar to the
critical u* value of 0.10 m s-1
found for CO2 fluxes at the same site (Hendriks et al., 2007).
CH4 flux data measured during periods with u* < 0.09 m s-1
occurred at 12% of the data
series and where removed too. The total amount of data gaps accounted for 26% of the
whole data series.
CH4 fluxes ánd CO2 fluxes (net ecosystem exchange (NEE)) were plotted for a two week
period in June 2006 at the Horstermeer site (Fig. 4.8). Although the CH4 fluxes are rather
variable over time, a diurnal cycle can be observed with low emission during the night and
high emission during the day. CO2 fluxes have a similar, but opposite, diurnal cycle. The
observed CH4 fluxes consisted mainly of emission and had an average of 29.7 nmol m-2
s-
1, while the typical maximum CH4 emission was approximately 80.0 nmol m
-2 s
-1. The
typical minimum flux was approximately 0.0 nmol m-2
s-1
and at three occasions a small
uptake was observed.
4.3.2 Intercomparison with flux chamber data
For two days during the CH4 eddy covariance measurement period at the Horstermeer site,
flux chamber measurements were made in the footprint of the eddy covariance tower with
a Photoacoustic Field Gas-Monitor (type 1312, Innova AirTech Instruments, Ballerup,
Denmark) connected with tubes to closed, dark chambers (Hendriks et al., 2007). Flux
chamber data were collected at the three land elements occurring in the footprint of the
eddy covariance tower: relatively dry peat land, saturated peat land and ditch water
surfaces. The fluxes from the various land elements are averaged with respect to their rela
tive surface area (70%, 20% and 10% respectively; Hendriks et al., 2007). On June 10 the
-20
-15
-10
-5
0
5
10
15
20
25
0 0.1 0.2 0.3 0.4
u* (m s-1
)
w'[C
H4
]' (n
mo
l m
-2 s
-1)
Figure 4.7: Results of
the analyses of the
effect of low turbulence
on nightly CH4 fluxes,
showing a drop in flux
magnitude below of u*
of 0.09 m s-1
. Data are
binned over u* classes
of 0.02 m s-1
and error
bars show the standard
deviation per class.
Chapter 4
84
flux chamber measurements showed an average CH4 flux of 114.5 ± 9.6 nmol m-2
s-1
,
while the eddy covariance measurements showed an average CH4 flux of 83.2 nmol m-2
s-1
over the same period (Fig. 4.9). On October 3 the average CH4 flux from the chamber
measurements was 53.6 ± 11.2 nmol m-2
s-1
, while that from eddy covariance was 61.6
nmol m-2
s-1
.
4.3.3 Simulation of alternative flux measurement approaches
The simulated 1Hz and disjunct eddy covariance data as well as the simulated REA data
were compared with the original 10Hz eddy covariance data as half hourly averages over a
15 day period (Table 4.2). It can be observed that the various methods show similar but
not identical results and that all alternative methods showed variations from the 10Hz
eddy covariance data (Fig. 4.10). The 1Hz eddy covariance method showed on average a
slight overestimation of the half hourly fluxes for CH4 measurements (2%) and the
standard deviation of the time series was somewhat higher than that of the 10Hz eddy
covariance. Average CO2 and water vapour fluxes determined with 1Hz eddy covariance
showed however a large underestimation compared to the 10Hz eddy covariance measure-
-30
-20
-10
0
10
20
30
176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191
time (julian days)
w'[C
O2]'
(µ
mol m
-2 s
-1)
-20
0
20
40
60
80
100
176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191
time (julian days)
w'[C
H4]'
(nm
ol m
-2 s
-1)
a.
b.
Figure 4.8: CH4 flux data series over a two week period in the summer of 2006 (a.) and CO2
flux (NEE) data series over the same period (b.).
An eddy covariance set-up for methane measurements
85
ements. The disjunct eddy covariance method showed on average a slight underestimation
of the half hourly fluxes for CH4 as well as for CO2 and water vapour measurements (-2%
and -3%), while the standard deviation was somewhat higher than that of the 10Hz eddy
covariance.
The b-value used in REA for correction of the deadband area was determined by Pattey et
al. (1993) as 0.56. For the measurement set-up investigated here, a b-value of 0.20 showed
results most similar to the normal 10Hz eddy covariance measurements for CH4
measurements as well as for CO2 and water vapour measurements. The results of the REA
method showed on average a small underestimation of the half hourly fluxes for CH4 as
well as for CO2 and water vapour measurements (-4% and -2%). The standard deviation
however, was significantly higher than that of the 10Hz eddy covariance, pointing at
relatively large deviations from the 10Hz measurements at a half hourly basis.
0
50
100
150
200
250
300
350
400
450
10:00 11:00 12:00 13:00 14:00 15:00
time-of-day
w'[C
H4]'
flu
x (
nm
ol m
-2 s
-1)
EC datadry landsaturated landditch water surface
average of flux chamber data
July 10 2006
flux chamber
measurements
0
50
100
150
200
250
300
350
400
10:00 11:00 12:00 13:00 14:00 15:00
time-of-day
w'[C
H4]'
(n
mol m
-2 s
-1)
EC data
dry land
saturated landditch water surface
average of flux chamber data
October 3 2006flux chamber
measurements
Figure 4.9: Hourly CH4
flux data at July 10 and
October 3 (both 2006)
plotted in combination
with flux chamber data
from various land
elements in the footprint
of the eddy covariance
tower collected at the
same day. The square
marks show the weighed
average of the flux
chamber measurements.
Chapter 4
86
CH4 flux (nmol m-2
s-2
) 26.74 27.35 26.29 25.76
CO2 flux (µmol m-2
s-2
) -6.53 -5.84 -6.31 -6.41
H2O flux (mmol m-2
s-2
) 3.13 2.79 3.05 3.01
CH4 flux (%) 0% 2% -2% -4%
CO2 flux (%) 0% -11% -3% -2%
H2O flux (%) 0% -11% -3% -4%
CH4 flux (nmol m-2
s-2
) 11.65 12.23 12.7 14.34
CO2 flux (µmol m-2
s-2
) 9.95 9.13 9.86 11.22
H2O flux (mmol m-2
s-2
) 2.82 2.59 2.8 2.77
average gas flux
average deviation
from normal 10Hz
eddy covariance
standard deviation
10Hz EC 1Hz ECDisjunct
1Hz EC
REA
(d=0.6;b=0.2)
Table 4.2: Summary of results of 1Hz eddy covariance, disjunct eddy covariance and REA
compared to 10Hz eddy covariance for CH4, CO2 and water vapour (H2O) flux
measurements. Average gas flux over the 15 day period, average deviation from the 10Hz
eddy covariance data and standard deviations of half hourly data are shown.
-10
0
10
20
30
40
50
179.5 179.6 179.7 179.8 179.9 180.0 180.1 180.2 180.3 180.4 180.5
time (julian days)
w'[C
H4]'
(n
mo
l m
-2 s
-1)
10Hz EC
1HZ EC
disjunct 1Hz EC
REA (d=0.6 and b=0.20)
Figure 4.10: Time series of CH4 fluxes for a one day period: half hourly averages of 10Hz
eddy covariance and simulated 1Hz eddy covariance, disjunct eddy covariance, and REA.
An eddy covariance set-up for methane measurements
87
4.4 Conclusions and discussion
The FMA, which uses the new off-axis ICOS technique, was found to perform
satisfactorily in laboratory experiments and in the eddy covariance field set-up. Compared
to other techniques, the absence of a large nitrogen Dewar for cooling that would need
weekly refill, the compact, narrow band and stable laser, the relative user friendliness and
low costs are considerable advantages. The FMA eddy covariance set-up was found to
perform independently in an unattended field situation. However, care should be taken
when placing the instrument with a scroll pump in the field. The FMA should be kept dry
and in ambient temperatures between 5oC and 45
oC, while the scroll pump should be kept
dry and cool. Contamination of the measurement cell should be prevented, since the
mirrors inside the measurement cell are sensitive and only a small contamination might
cause a rapid decrease in reflectivity of the mirrors and performance of the instrument.
The analysis of the Allan variance indicated a high precision and system stability of the
FMA. Additionally, the calibration experiment showed sufficiently high accuracy (< 0.30
%). As long as ambient temperatures do not exceed the range of 5 to 45 oC and pressure in
the measurement cell is near 210 hPa, the CH4 measurements are not affected by changes
in Tcell and Pcell. Since no instrumental drift was observed in the Allan variance analyses, in
the calibration experiment or in the comparison with CH4 concentration data at a field site
nearby, it was concluded that frequent calibration of the FMA was not necessary.
The observed τ was 0.10 s, implying a maximum sampling rate of 10Hz which is
sufficient for eddy covariance measurements. The closed path FMA eddy covariance
system performed well, as shown by the power- and co-spectra which corresponded well
to the theoretical spectral curves. Additionally, the energy balance showed satisfactory
closure. CH4 fluxes appeared to be underestimated during periods with low turbulence and
a u* correction was applied for CH4 flux data during periods with u* < 0.09 m s-1
. Due to
erroneous measurements, spikes and periods of low turbulence the data series consisted
for 26% of gaps.
Observed CH4 fluxes consisted mainly of emission, showed a diurnal cycle, but were
rather variable over time. The average CH4 emission was 29.7 nmol m-2
s-1
, while the
typical maximum CH4 emission was approximately 80.0 nmol m-2
s-1
and the typical
minimum flux was approximately 0.0 nmol m-2
s-1
. These CH4 fluxes were in agreement
with QCL flux measurements at a managed peat meadow site in the Netherlands
(Reeuwijk), where emissions were 40 ± 31 nmol m-2
s-1
on average (Kroon et al., 2007)
and average annual CH4 emission of 30 nmol m-2
s-1
from peat lands in Germany and the
Netherlands (Drösler et al., 2007). From the comparison of the eddy covariance
measurements with flux chamber measurements, it was observed that the fluxes from the
two techniques showed a discrepancy of approximately 20%. However, considering the
fact that the flux chamber measurements are point measurements at the soil surface while
the eddy covariance has a footprint of hundreds of square meters, some degree of variation
may be expected.
Additionally, raw CH4, CO2 and water vapour 10Hz field data were manipulated to
simulate 1Hz eddy covariance, disjunct eddy covariance and REA. It was concluded that,
Chapter 4
88
when using a scroll pump is not possible for technical or practical reasons; disjunct eddy
covariance was the most reliable substitute for 10Hz eddy covariance. This method
showed the highest degree of resemblance with the 10Hz eddy covariance for all three
gases. The simulated 1Hz eddy covariance of CO2 and water vapour fluxes, showed
relatively large deviations from the 10Hz eddy covariance data, indicating a reduced
reliability of the method and no possibility to test the validity of the method at sites
without the eddy covariance set-up for CH4. Simulation of REA did show similar results
for all three gases; however, the standard deviation of the time series was significantly
higher than that of the 10Hz eddy covariance, pointing at relatively large deviations from
the 10Hz measurements at the half hourly basis. REA was therefore evaluated to generate
reliable estimates of fluxes over periods in the order of days or weeks. Importantly, the b-
value for CH4 flux measurements was the same as that for the CO2 and water vapour flux
measurements. This indicates that it will be possible to determine the b-value for CH4
measurements with REA at new and remote locations using an eddy covariance set-up
with low power requirements for CO2 or water vapour. Finally, it should be taken into
account that the ‘snap sampling’ instrument for disjunct eddy covariance and the valve
switching system for REA will introduce additional artefacts, which also require certain
amounts of power (Rinne et al., 2000; Kuhn et al., 2005; Graus et al., 2006).
Acknowledgements
This research project is performed in the framework of the European research programme
Carbo Europe (contract number GOCE-CT2003-505572) and the Dutch National
Research Programme Climate Changes Spatial Planning (www.klimaatvooruimte.nl). We
very much appreciate the help from Alex Vermeulen working at ECN for the information
and data from the Cabauw site. Also, we would very much like to thank our technical co-
operators Rob Stoevelaar and Ron Lootens.
An eddy covariance set-up for methane measurements
89
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